References quoted in the XUNDL dataset: 16O 15N(7LI,6HE):XUNDL-44
7 references found.
Clicking on a keynumber will list datasets that reference the given article.
J.Phys.(Paris) 34, 363 (1973)
F.Brochard, P.Chevallier, D.Disdier, V.Rauch, F.Scheibling
Etude des Desexcitations Electromagnetiques des Niveaux 1- Situes a 12.44 et 13.09 MeV dans le Noyau 16O
NUCLEAR REACTIONS 12C(α, γ), E=7.05 MeV; measured Eγ. 16O levels deduced transitions, J, π.
Z.Phys. A305, 325 (1982)
A.Redder, H.W.Becker, H.Lorenz-Wirzba, C.Rolfs, P.Schmalbrock, H.P.Trautvetter
The 15N(p, α0)12C Reaction at Stellar Energies
NUCLEAR REACTIONS 15N(p, α), E=78-810 keV; measured σ(E, θ); deduced astrophysical S-factor. 16O resonances deduced Γ, Γp, Γα.
Phys.Rev. C 76, 065804 (2007)
M.La Cognata, S.Romano, C.Spitaleri, S.Cherubini, V.Crucilla, M.Gulino, L.Lamia, R.G.Pizzone, A.Tumino, R.Tribble, C.Fu, V.Z.Goldberg, A.M.Mukhamedzhanov, D.Schmidt, G.Tabacaru, L.Trache, B.F.Irgaziev
Astrophysical S(E) factor of the 15N(p, α)12C reaction at sub-Coulomb energies via the Trojan horse method
NUCLEAR REACTIONS 2H(15N, nα), E=60 MeV; measured 12C energies, particle coincidences, momentum. 15N(p, α)12C, E(cm)=19.2-576.0 MeV; deduced angular distributions, excitation functions, astrophysical S-factors using Trojan horse method.
doi: 10.1103/PhysRevC.76.065804
Phys.Rev. C 82, 055804 (2010), Erratum Phys.Rev. C 84, 019902 (2011)
P.J.LeBlanc, G.Imbriani, J.Gorres, M.Junker, R.Azuma, M.Beard, D.Bemmerer, A.Best, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, M.Couder, R.deBoer, Z.Elekes, S.Falahat, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, F.Kappeler, A.Kontos, R.Kuntz, H.Leiste, A.Lemut Q.Li, B.Limata, M.Marta, C.Mazzocchi, R.Menegazzo, S.O'Brien, A.Palumbo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, E.Stech, O.Straniero, F.Strieder, W.Tan, F.Terrasi, H.P.Trautvetter, E.Uberseder, M.Wiescher
Constraining the S factor of 15N(p, γ)16O at astrophysical energies
NUCLEAR REACTIONS 15N(p, γ), E=130-1800 keV; measured Ep, Ip, Eγ, Iγ, σ(E), σ(θ); deduced resonances, branching ratios, astrophysical S factors and reaction rates. Multilevel R-matrix analysis. Implications for the first and second cycles of the CNO cycles.
doi: 10.1103/PhysRevC.82.055804
Phys.Rev. C 85, 065810 (2012), Erratum Phys.Rev. C 86, 039902 (2012)
G.Imbriani, R.J.de Boer, A.Best, M.Couder, G.Gervino, J.Gorres, P.J.LeBlanc, H.Leiste, A.Lemut, E.Stech, F.Strieder, E.Uberseder, M.Wiescher
Measurement of γ rays from 15N(p, γ)16O cascade and 15N(p, α1γ)12C reactions
NUCLEAR REACTIONS 15N(p, γ)16O, 15N(p, αγ)12C, E=0.14-1.80 MeV; measured Eγ, Iγ, S factors, cross section. 12C, 16O; deduced levels, J, π, widths. R-matrix analysis. Comparison with previous studies.
doi: 10.1103/PhysRevC.85.065810
Rev.Mod.Phys. 89, 035007 (2017)
R.J.deBoer, J.Gorres, M.Wiescher, R.E.Azuma, A.Best, C.R.Brune, C.E.Fields, S.Jones, M.Pignatari, D.Sayre, K.Smith, F.X.Timmes, E.Uberseder
The 12C(α, γ)16O reaction and its implications for stellar helium burning
NUCLEAR REACTIONS 12C(α, γ)16O, E(cm)<6 MeV; analyzed available data; deduced σ, reaction rates and uncertainties.
doi: 10.1103/RevModPhys.89.035007
Phys.Rev. C 112, 045802 (2025)
C.Chen, Y.J.Li, Z.H.Li, Y.Zhang, J.W.Tian, J.Y.H.Li, Y.Q.Zhang, C.Dong, F.Q.Cao, J.C.Liu, Q.W.Fan, E.T.Li, S.Q.Yan, Y.B.Wang, S.Zeng, G.Lian, W.Nan, N.Song, D.Nan
Indirect measurement of the astrophysical reaction rates of 15N(p, γ)16O
NUCLEAR REACTIONS 15N(7Li, 6He), E=44 MeV; measured reaction products; deduced σ(θ), the proton asymptotic normalization coefficient (ANC), S factor, resonance parameters with R-matrix analysis. Comparison with available data. The Q3D magnetic spectrometer at the HI-13 tandem accelerator of the China Institute of Atomic Energy in Beijing.
doi: 10.1103/rvss-98yr